- Timestamp:
- 01/25/05 22:15:23 (20 years ago)
- Location:
- trunk/MagicSoft/GRB-Proposal
- Files:
-
- 4 edited
Legend:
- Unmodified
- Added
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trunk/MagicSoft/GRB-Proposal/Introduction.tex
r5968 r6000 48 48 GRB, TIME DEVELOPMENT, EXPECTED FLUXES, SPECTRA } \ldots 49 49 \par 50 \ldots {\bf UPDATE CURRENT PAPERS} \ldots 51 \par 52 \par 53 \ldots {\bf MORE DETAILED DESCRIPTION OF GEV-EMISSION MODELS }\ldots 54 \par 55 \par 56 \ldots {\bf SATOKO AND MARKUS GARCZ.}\ldots 57 \par 50 58 In the year 2005, three satellites will produce GRB alerts: The \he 51 59 satellite, launched in October 2000, the \ig satellite, launched October 2002 and the -
trunk/MagicSoft/GRB-Proposal/Monitor.tex
r5968 r6000 1 1 \section{The GRB monitor at La Palma} 2 2 3 \subsection{The socket connection to GCN} 4 \subsection{The GRB webpage} 5 \subsection{The accoustic alert} 6 \subsection{The interface to the Central Control} 7 \subsection{Emails to the GRB-mailing list} 8 9 3 10 \ldots {\bf NICOLA } \ldots -
trunk/MagicSoft/GRB-Proposal/Strategies.tex
r5968 r6000 1 1 \section{Proposed Observation Strategies} 2 2 3 \ldots {\bf PRODUCE A PLOT WITH THE OVERLAP BETWEEN SWIFT AND MAGIC } \ldots 3 \ldots {\bf PRODUCE A PLOT WITH THE OVERLAP BETWEEN SWIFT AND MAGIC-- Markus Garcz. } \ldots 4 5 \ldots {\bf PRODUCE PLOT WITH ESTIMATION OF MAX. ZENITH ANGLE DEP. ON GAMMA-RAY HORIZON } \ldots 4 6 5 7 \ldots {\bf SIMULATE BURTS AND TRIGGER THEM WITH SWIFT AND MAGIC } \ldots … … 11 13 \subsection{What to do with moon shine ? } 12 14 13 \ldots {\bf NICOLA, HV TABLES ...} \ldots15 \ldots {\bf NICOLA, HV TABLES, LIDS ... -- CAMERA EXPERTS - ECKART, RAZMIK, MANEL, JOSE} \ldots 14 16 15 \subsection{ What to do with camera?}17 \subsection{Calibration } 16 18 17 \ldots {\bf LIDS OPEN ...} \ldots19 \ldots {\bf MARKUS gAUG} \ldots 18 20 -
trunk/MagicSoft/GRB-Proposal/Timing.tex
r5968 r6000 9 9 10 10 The EGRET~\cite{EGRET} instrument on the CGRO 11 has detected GeV emission of GRB940217 promptly and 90 sec. after11 has detected GeV emission of GRB940217 promptly and 90 min. after 12 12 the burst onset. 13 13 \\ … … 22 22 UHE component with radiation maxima of up to one day or even one week (accompanied by long-term 23 23 neutrino emission). 24 25 \par 26 \ldots \textit{\bf UNTIL WHEN WILL WE OBSERVE THE BURST AFTER OCCURRANCE} \ldots 27 \par
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